Development and Parameters of a Non-Self-Similar CME Caused by Eruption of a Quiescent Prominence
I.V. Kuzmenko (1), V.V. Grechnev (2) ((1) Ussuriysk Astrophysical, Observatory, Russia, (2) Institute of Solar-Terrestrial Physics SB RAS,, Irkutsk, Russia)

TL;DR
This study analyzes a 2013 quiescent prominence eruption and associated CME, revealing non-self-similar expansion, prominence-driven mass supply, and structural evolution into a flux rope, using multi-instrument observations and modeling.
Contribution
It provides detailed parameters and kinematic analysis of a non-self-similar CME driven by a quiescent prominence eruption, highlighting structural changes and mass transfer processes.
Findings
CME mass mainly supplied by the prominence (~6×10^15 g)
CME expansion was not self-similar up to 25 R⊙
Structural transformation into a flux rope observed during expansion
Abstract
The eruption of a large quiescent prominence on 17 August 2013 and associated coronal mass ejection (CME) were observed from different vantage points by Solar Dynamics Observatory (SDO), Solar-Terrestrial Relations Observatory (STEREO), and Solar and Heliospheric Observatory (SOHO). Screening of the quiet Sun by the prominence produced an isolated negative microwave burst. We estimated parameters of the erupting prominence from a model of radio absorption and measured from 304 \AA\ images. Their variations obtained by both methods are similar and agree within a factor of two. The CME development was studied from the kinematics of the front and different components of the core and their structural changes. The results are verified using movies in which the CME expansion was compensated according to the measured kinematics. We found that the CME mass ( g) was mainly…
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